核心坍缩超新星爆发机制：状态报告
天体物理学
2009-11-07 v1
摘要
我们综述了当前寻找理解核心坍缩超新星机制的进展，若以 neutrino 驱动为例。在此过程中，我们讨论了球对称爆发范式及其问题，来自我们新套套件的坍缩计算结果，其使用了刚开发展的 1D 隐式、多组、Feautrier/切向射线、Boltzmann 求解器耦合到显式预测/正确子流体力学，超新星爆发的基本能量动力学，以及多维辐射/流体模拟的前景，以解释巨型恒星核心为何爆发。
引用
@article{arxiv.astro-ph/0210212,
title = {The Mechanism of Core-Collapse Supernova Explosions: A Status Report},
author = {Adam Burrows and Todd A. Thompson},
journal= {arXiv preprint arXiv:astro-ph/0210212},
year = {2009}
}
备注
10 pages, LaTeX, 4 JPEGs included. To be published in the proceedings to the ESO/MPA/MPE Workshop (an ESO Astrophysics Symposium) entitled "From Twilight to Highlight: The Physics of Supernovae," held in Garching bei M\"unchen, Germany, July 29-31, 2002, eds. Bruno Leibundgut and Wolfgang Hillebrandt (Springer-Verlag)